Black hole size and phase space volumes
Samir D. Mathur
TL;DR
The paper argues that extremal black holes in string theory are best described as horizonless fuzzballs whose boundary areas scale with the enclosed microstate entropy, thereby linking geometric size to phase-space volume. By analyzing the NS1-P and its D1-D5 duals, Mathur shows that for the 2-charge system the boundary area satisfies a relation of the form $${A_E^{(10)}}/{G_N^{(10)}} \sim S_{micro}$, and extends the analysis to sub-ensembles where the entropy is reduced by a factor $M$ with a corresponding $1/M$ reduction in boundary area. It also applies the same reasoning to the rotating 2-charge black ring, obtaining $${A_E^{(10)}}/{G_N^{(10)}} \sim \sqrt{n'_1 n'_5 - J}$ for the full ensemble and $\sim (1/M)\sqrt{n'_1 n'_5 - J}$ for sub-ensembles. The work further analyzes quantum corrections, finding that string 1-loop effects ($R^4$ terms) remain small at the fuzzball boundary for a wide range of the sub-ensemble parameter $M$, supporting the robustness of the leading area-entropy relation. Altogether, the paper argues that phase-space considerations underpin the fuzzball geometry and suggests connections to holography and other entropy formalisms, potentially guiding understanding of black hole microstates in more general charge configurations.
Abstract
For extremal black holes the fuzzball conjecture says that the throat of the geometry ends in a quantum `fuzz', instead of being infinite in length with a horizon at the end. For the D1-D5 system we consider a family of sub-ensembles of states, and find that in each case the boundary area of the fuzzball satisfies a Bekenstein type relation with the entropy enclosed. We suggest a relation between the `capped throat' structure of microstate geometries and the fact that the extremal hole was found to have zero entropy in some gravity computations. We examine quantum corrections including string 1-loop effects and check that they do not affect our leading order computations.
